We have previously shown [1]} that the shadow of Sgr A* is enlarged in EQG by an amount less than 10 nanoarcseconds relative to GR for \(K/M_{Sgr A*}^{6}\approx 2.21\times 10^{-1}\) .
This occurs because the size of the shadow of Sgr A* is of order of \(10^{-5}\)  arcseconds whether or not its gravitational field is governed by GR or EQG, and is far lower than the resolution of today's observational facilities such as Event Horizon Telescope [2]}, [3]}.
